{"record_type":"pith_number_record","schema_url":"https://pith.science/schemas/pith-number/v1.json","pith_number":"pith:2006:TRPWLXYDOST2HGBUCL56BU3N3W","short_pith_number":"pith:TRPWLXYD","schema_version":"1.0","canonical_sha256":"9c5f65df0374a7a3983412fbe0d36ddd9f6a48836e0f1d6d0bdaa146dc8b1152","source":{"kind":"arxiv","id":"astro-ph/0612779","version":1},"attestation_state":"computed","paper":{"title":"On the structure of the turbulent interstellar atomic hydrogen. II- First comparison between observation and theory","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Audit, M.-A Miville-Deschenes, P. Hennebelle","submitted_at":"2006-12-29T15:20:33Z","abstract_excerpt":"{It is necessary to understand the dynamics of the atomic gas to use complex modeling and to carry out detailed comparisons between theoretical models and observations.}{In a companion paper, we present high resolution bidimensional numerical simulations of the interstellar atomic hydrogen. Here, we further characterize these simulations and we compare our results with various observations.}{We give statistics of the column density and velocity along the line of sight and show that they compare favorably with observations of high-latitude lines of sight. We compute synthetic HI spectra and qua"},"verification_status":{"content_addressed":true,"pith_receipt":true,"author_attested":false,"weak_author_claims":0,"strong_author_claims":0,"externally_anchored":false,"storage_verified":false,"citation_signatures":0,"replication_records":0,"graph_snapshot":true,"references_resolved":false,"formal_links_present":false},"canonical_record":{"source":{"id":"astro-ph/0612779","kind":"arxiv","version":1},"metadata":{"license":"","primary_cat":"astro-ph","submitted_at":"2006-12-29T15:20:33Z","cross_cats_sorted":[],"title_canon_sha256":"a17e1f3703b9cee99735f90497fd1ff3a4375a483ac9f19bf8f6b45c2a3b92fd","abstract_canon_sha256":"2e441bce0188b7cf539e2301364ece69d4c086a03846ab6a0c26d89953ce9b47"},"schema_version":"1.0"},"receipt":{"kind":"pith_receipt","key_id":"pith-v1-2026-05","algorithm":"ed25519","signed_at":"2026-07-04T14:58:17.529362Z","signature_b64":"BwmoOg6nz9CT4EJsXoCON71uZFtUuQZue35KyisxvUxLxfv9vArMAv6NeMCvzTG6xO/f16UcQaGxFIo3uI+IAQ==","signed_message":"canonical_sha256_bytes","builder_version":"pith-number-builder-2026-05-17-v1","receipt_version":"0.3","canonical_sha256":"9c5f65df0374a7a3983412fbe0d36ddd9f6a48836e0f1d6d0bdaa146dc8b1152","last_reissued_at":"2026-07-04T14:58:17.529000Z","signature_status":"signed_v1","first_computed_at":"2026-07-04T14:58:17.529000Z","public_key_fingerprint":"8d4b5ee74e4693bcd1df2446408b0d54"},"graph_snapshot":{"paper":{"title":"On the structure of the turbulent interstellar atomic hydrogen. II- First comparison between observation and theory","license":"","headline":"","cross_cats":[],"primary_cat":"astro-ph","authors_text":"E. Audit, M.-A Miville-Deschenes, P. Hennebelle","submitted_at":"2006-12-29T15:20:33Z","abstract_excerpt":"{It is necessary to understand the dynamics of the atomic gas to use complex modeling and to carry out detailed comparisons between theoretical models and observations.}{In a companion paper, we present high resolution bidimensional numerical simulations of the interstellar atomic hydrogen. Here, we further characterize these simulations and we compare our results with various observations.}{We give statistics of the column density and velocity along the line of sight and show that they compare favorably with observations of high-latitude lines of sight. We compute synthetic HI spectra and qua"},"claims":{"count":0,"items":[],"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"source":{"id":"astro-ph/0612779","kind":"arxiv","version":1},"verdict":{"id":null,"model_set":{},"created_at":null,"strongest_claim":"","one_line_summary":"","pipeline_version":null,"weakest_assumption":"","pith_extraction_headline":""},"integrity":{"clean":true,"summary":{"advisory":0,"critical":0,"by_detector":{},"informational":0},"endpoint":"/pith/astro-ph/0612779/integrity.json","findings":[],"available":true,"detectors_run":[],"snapshot_sha256":"c28c3603d3b5d939e8dc4c7e95fa8dfce3d595e45f758748cecf8e644a296938"},"references":{"count":0,"sample":[],"resolved_work":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57","internal_anchors":0},"formal_canon":{"evidence_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"author_claims":{"count":0,"strong_count":0,"snapshot_sha256":"258153158e38e3291e3d48162225fcdb2d5a3ed65a07baac614ab91432fd4f57"},"builder_version":"pith-number-builder-2026-05-17-v1"},"aliases":[{"alias_kind":"arxiv","alias_value":"astro-ph/0612779","created_at":"2026-07-04T14:58:17.529061+00:00"},{"alias_kind":"arxiv_version","alias_value":"astro-ph/0612779v1","created_at":"2026-07-04T14:58:17.529061+00:00"},{"alias_kind":"doi","alias_value":"10.48550/arxiv.astro-ph/0612779","created_at":"2026-07-04T14:58:17.529061+00:00"},{"alias_kind":"pith_short_12","alias_value":"TRPWLXYDOST2","created_at":"2026-07-04T14:58:17.529061+00:00"},{"alias_kind":"pith_short_16","alias_value":"TRPWLXYDOST2HGBU","created_at":"2026-07-04T14:58:17.529061+00:00"},{"alias_kind":"pith_short_8","alias_value":"TRPWLXYD","created_at":"2026-07-04T14:58:17.529061+00:00"}],"events":[],"event_summary":{},"paper_claims":[],"inbound_citations":{"count":0,"internal_anchor_count":0,"sample":[]},"formal_canon":{"evidence_count":0,"sample":[],"anchors":[]},"links":{"html":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W","json":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W.json","graph_json":"https://pith.science/api/pith-number/TRPWLXYDOST2HGBUCL56BU3N3W/graph.json","events_json":"https://pith.science/api/pith-number/TRPWLXYDOST2HGBUCL56BU3N3W/events.json","paper":"https://pith.science/paper/TRPWLXYD"},"agent_actions":{"view_html":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W","download_json":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W.json","view_paper":"https://pith.science/paper/TRPWLXYD","resolve_alias":"https://pith.science/api/pith-number/resolve?arxiv=astro-ph/0612779&json=true","fetch_graph":"https://pith.science/api/pith-number/TRPWLXYDOST2HGBUCL56BU3N3W/graph.json","fetch_events":"https://pith.science/api/pith-number/TRPWLXYDOST2HGBUCL56BU3N3W/events.json","actions":{"anchor_timestamp":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W/action/timestamp_anchor","attest_storage":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W/action/storage_attestation","attest_author":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W/action/author_attestation","sign_citation":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W/action/citation_signature","submit_replication":"https://pith.science/pith/TRPWLXYDOST2HGBUCL56BU3N3W/action/replication_record"}},"created_at":"2026-07-04T14:58:17.529061+00:00","updated_at":"2026-07-04T14:58:17.529061+00:00"}